Andromache (PBK) - download pdf or read online
By Euripides, P. T. Stevens
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Reproduced by permission of the AAS from Fitzpatrick, E. , and Massa, D. 2007. 5. The Horsehead Nebula (left) optical image from the VLT (ESO) and (right) the JCMT-SCUBA 850 µm contour map. The bright submillimetre regions indicate emission from prestellar objects. , and Attwood, R. 2006. ) Although the chemical nature and physical structure of the dust are undoubtedly important for all these topics, we do not discuss them here. We do not describe other dust properties, nor the origin of dust in supernovae, novae, and other stellar winds, but simply refer to relevant works on the subject (see Further Reading).
Evidently, nitrogen does not follow the pattern of oxygen; neither does sulfur. However, by creating the first products of oxygen and carbon chemistry, cosmic rays open the door to a more complex chemistry, because these first products may interact with atoms and ions to form new products. For example, exchange reactions of OH with O, C, N, and S create O2 , CO, NO, and SO, respectively. Exchange reactions of CH with the same set of atoms create CO, C2 , CN, and CS. 34 3 Astrochemical Processes Higher levels of chemical complexity can be attained by reactions involving these second-rank products, either among themselves or with existing atoms and ions, to form third-rank products.
Eds. New York: Oxford University Press. Tennyson, J. 2005. Astronomical Spectroscopy: An Introduction to the Atomic and Molecular Physics of Astronomical Spectra. London: Imperial College Press. 1 What Drives Cosmic Chemistry? It is a relatively straightforward matter to use freely available computer codes and lists of chemical reactions to compute abundances of molecular species for many types of interstellar or circumstellar region. For example, the UDfA, Ohio, and KIDA websites (see Chapter 9) provide lists of relevant chemical reactions and reaction rate data.
Andromache (PBK) by Euripides, P. T. Stevens